X-Ray Observations of the Galactic Center with Suzaku(Chapter 5. The Galactic Center and Ridge Emissions, The Extreme Universe in the Suzaku Era)
スポンサーリンク
概要
- 論文の詳細を見る
The diffuse X-ray emissions from the Galactic center (GCDX) are observed with the X-ray Imaging Spectrometer (XIS) on Suzaku. The high-energy resolution and the low-background orbit provide excellent spectra of the GCDX. The results of the Galactic center (GC) observations are; (1) the origin of the 6.7/7.0keV lines is not a charge exchange process, but is collisional excitation in hot plasma, (2) the majority of the X-ray emission is not an integrated flux of unresolved point sources, but is diffuse, (3) new SNR candidates are found and (4) the 6.4keV line is not fluorescence by electrons but by X-rays.
- 理論物理学刊行会の論文
- 2007-12-19
著者
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Koyama Katsuji
Department Of Physics Kyoto University
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Koyama Katsuji
Department Of Astrophysics School Of Science Nagoya University
関連論文
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